Slater Insulator in Iridate Perovskites with Strong Spin-Orbit Coupling

Q. Cui, J.-G. Cheng, W. Fan, A. E. Taylor, S. Calder, M. A. McGuire, J.-Q. Yan, D. Meyers, X. Li, Y. Q. Cai, Y. Y. Jiao, Y. Choi, D. Haskel, H. Gotou, Y. Uwatoko, J. Chakhalian, A. D. Christianson, S. Yunoki, J. B. Goodenough, and J.-S. Zhou
Phys. Rev. Lett. 117, 176603 – Published 20 October 2016
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Abstract

The perovskite SrIrO3 is an exotic narrow-band metal owing to a confluence of the strengths of the spin-orbit coupling (SOC) and the electron-electron correlations. It has been proposed that topological and magnetic insulating phases can be achieved by tuning the SOC, Hubbard interactions, and/or lattice symmetry. Here, we report that the substitution of nonmagnetic, isovalent Sn4+ for Ir4+ in the SrIr1xSnxO3 perovskites synthesized under high pressure leads to a metal-insulator transition to an antiferromagnetic (AF) phase at TN225K. The continuous change of the cell volume as detected by x-ray diffraction and the λ-shape transition of the specific heat on cooling through TN demonstrate that the metal-insulator transition is of second order. Neutron powder diffraction results indicate that the Sn substitution enlarges an octahedral-site distortion that reduces the SOC relative to the spin-spin exchange interaction and results in the type-G AF spin ordering below TN. Measurement of high-temperature magnetic susceptibility shows the evolution of magnetic coupling in the paramagnetic phase typical of weak itinerant-electron magnetism in the Sn-substituted samples. A reduced structural symmetry in the magnetically ordered phase leads to an electron gap opening at the Brillouin zone boundary below TN in the same way as proposed by Slater.

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  • Received 18 May 2016

DOI:https://doi.org/10.1103/PhysRevLett.117.176603

© 2016 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Q. Cui1, J.-G. Cheng1,2,*, W. Fan3, A. E. Taylor4, S. Calder4, M. A. McGuire5, J.-Q. Yan5,6, D. Meyers7, X. Li2, Y. Q. Cai2, Y. Y. Jiao1, Y. Choi8, D. Haskel8, H. Gotou9, Y. Uwatoko9, J. Chakhalian10, A. D. Christianson4,11, S. Yunoki3,12,13, J. B. Goodenough2, and J.-S. Zhou2,†

  • 1Beijing National Laboratory for Condensed Matter Physics and Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China
  • 2Materials Science and Engineering Program, University of Texas at Austin, Austin, Texas 78712, USA
  • 3Computational Condensed Matter Physical Laboratory, RIKEN, Wako, Saitama 351-0198, Japan
  • 4Quantum Condensed Matter Division, Oak Ridge National Laboratory, Tennessee 37831, USA
  • 5Materials Science and Technology Division, Oak Ridge National Laboratory, Tennessee 37831, USA
  • 6Department of Materials Science and Engineering, University of Tennessee, Knoxville, Tennessee 37996, USA
  • 7Department of Physics, University of Arkansas, Fayetteville, Arkansas 72701, USA
  • 8Advanced Photon Source, Argonne National Laboratory, Argonne, Illinois 60439, USA
  • 9Institute for Solid State Physics, University of Tokyo, 5-1-5 Kashiwanoha, Chiba 277-8581, Japan
  • 10Department of Physics and Astronomy, Rutgers University, 136 Frelinghuysen Road, Piscataway, New Jersey 08854, USA
  • 11Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37966, USA
  • 12Computational Materials Science Research Team, RIKEN Advanced Institute for Computational Science (AICS), Kobe, Hyogo 650-0047, Japan
  • 13Computational Quantum Matter Research Team, RIKEN Center for Emergent Matter Science (CEMS), Wako, Saitama 351-0198, Japan

  • *jgcheng@iphy.ac.cn
  • jszhou@mail.utexas.edu

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Issue

Vol. 117, Iss. 17 — 21 October 2016

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